Doppler Shift Oscillations of Hot Solar Coronal Plasma Seen by SUMER: A Signature of Loop Oscillations?

By Tongjiang Wang, S. Solanki, W. Curdt, D. Innes, I. Dammasch. 2002

219 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/5658263507c24ae6113ba41c622a8dc0665bc421

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

Citations in the corpus

Rapid Acceleration of a Coronal Mass Ejection in the Low Corona and Implications for Propagation (2003, background): “This is then followed at 00:44:53 UT by a linear jetlike feature emerging from close to the westernmost footpoint (Wang et al. 2002).”
Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, unknown): “Longitudinal oscillations in coronal loops were discovered as periodic Doppler shifts recorded with the SOHO/SUMER instrument (Wang et al. 2002), and hence are often called SUMER oscillations.”
Vertical oscillations of a coronal loop observed by TRACE (2004, methodology): “Later, hot loop oscillations in Doppler shifts with periods on the order of 20 min were detected by the SUMER spectrometer onboard SOHO, and interpreted in terms of the standing slow mode (e.g. Wang et al. 2002, 2003; Ofman & Wang 2002).”
Coronal Waves and Oscillations (2005, background): “, 2002), and longitudinal standing oscillations within loops (Kliem et al., 2002; Wang et al., 2002).”
Hot Coronal Loop Oscillations Observed by SUMER: Slow Magnetosonic Wave Damping by Thermal Conduction (2002, methodology): “The parameters of the time series for 35 oscillations in 17 events were derived and are given by Wang et al. (2002c).”
The EUV Imaging Spectrometer for Hinode (2007, background): “Spectroscopic observations of oscillations in coronal loops have been made in flaring and post flare conditions (Wang et al., 2002, 2003), while on a larger scale spectroscopic observations of EIT waves in the corona have been pioneered by Harra and Sterling (2003).”
Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, methodology): “Their first direct evidence was provided by Wang et al. (2002) using a high-resolution imaging spectrometer, SUMER, onboard SOHO.”
Global sausage modes of coronal loops (2003, background): “The particular examples are global (or standing, with the wave length equal to double the length of the loop) kink modes (Aschwanden et al. 1999; Nakariakov et al. 1999) and standing longitudinal (slow magnetoacoustic) modes (Wang et al. 2002; Ofman & Wang 2002).”
CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, background): “…(Roberts et al. 1984; Asai et al. 2001; Melnikov et al. 2002; Aschwanden et al. 2004), slow (acoustic) mode oscillations with SUMER/SOHO (Wang et al. 2002; Kliem et al. 2002), slow (acoustic) propagating waves with UVCS/SOHO (Ofman et al. 1997) and Hinode (Erdelyi & Taroyan 2008),…”
Slow-mode standing waves observed by SUMER in hot coronal loops (2003, methodology): “Very recently, the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer on SOHO discovered damped oscillations of hot coronal loops in Doppler shift (Kliem et al. 2002; Wang et al. 2002a–c, 2003).”
Hot coronal loop oscillations observed with SUMER: Examples and statistics (2003, methodology): “07±0.16) obtained on the basis of data for 35 cases by Wang et al. (2002c).”